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Desert Sky Observer Volume 35 Antelope Valley Astronomy Club Newsletter March 2015 Up-Coming Events
March 7: Prime Desert Moon Walk March 13: Club Meeting* March 21: Messier Marathon March 25: Acton Library Star Party
* Monthly meetings are held at the S.A.G.E. Planetarium in Palmdale, the second Friday of each month. The meeting location is at the northeast corner of Avenue R and 20th Street East. Meetings start at 7 p.m. and are open to the public. Please note that food and drink are not allowed in the planetarium
President Frank Moore
Winter astronomy strikes again. For those of you who missed it, and quite a few did, on February 21 we had our February Dark Sky Star Party at the Antelope Valley California Poppy Reserve. The hearty souls who attended braved cold temperatures and a biting
wind to set up and view the cosmos. Because of the threat of rain Matt Leone brought his 16” dob, in lieu of his 24”, as it afforded easier and
faster take down if we had to make a retreat. Darrell Bennett had his 12” Meade SCT, Rose and Frank Moore their Celestron C-11, and Ellen Mahler her 6” Orion dob. The other brave souls in attendance included Ruth Olson, Inga Nagel, and Bob Gauldin. Bob Ayres brought his SCT and mount but as it was near dark when he arrived, and already biting cold, he held in abeyance in his truck while we waited, and hoped, the weather would improve. It didn’t.
Though clouds were threatening on the horizons, especially to the south, views were crystal clear in the open parts of the sky. The performance of the night was put on by Venus and Mars, which were half a degree apart as they descended in the western sky. To the north, in Ursa Major, the sky containing M81/M82, Bode’s and the Cigar Galaxies, was clear throughout the night and the pair were clearly visible together in wider field eyepieces. Other objects in the their group offered satisfying views between the gusts of wind as well. Still, conditions were challenging, and with the gusting wind stars sometimes appeared to be figure eights or infinity signs instead of pinpricks of light in the eyepieces.
The weather forecast had called for the wind to die down by 8:00 and, when it hadn’t, and the clouds began to move in from the south, we all made the collective decision to call it night by 9:00 pm.
Events coming up in March include the monthly Moon Walk and public observing at Prime Desert Woodland Preserve on Saturday March 7 at 6:30 pm, the club meeting at the SAGE Planetarium on Friday March 13, and our annual Messier Marathon at Saddleback Butte State Park on March 21. We have the group site at Saddleback Butte reserved from 2:00 pm on March 21 till 8:00 am on March 22. Let’s all think good thoughts and hope for better weather for the Messier Marathon.
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Stay tuned for announcements and watch the calendar, as April will be a busy month as well. We have a lunar eclipse in the early morning hours of Saturday April 4, a Beginner’s Astronomy Class at 2:00 pm at the SAGE and Prime Desert Woodland Moon Walk at 7:45pm on Saturday April 11, and our booth at the California Poppy Festival on Saturday and Sunday April 18 and 19. We’ll also be supporting the Edwards Air Force Base Youth “Lock-In” with a star party on Friday April 24. Watch for times and sign up information on these events.
Remember to support our sponsors as they help make our activities and public outreach possible. Wishing us all clear skies for the rest our annual events.
Vice President Don Bryden
March is upon us! This weekend we have a PDW outing (if the skies clear!) and of course the monthly meeting. We’re still hoping for a speaker from Griffith Observatory but as of yet it is not final. Still, we’ll have a nice dome show and several raffles and then Jeremy can give us a tour of the night sky. We’ll have information on the Lunar eclipse on
April 4th and the Messier Marathon on the 21st of March at Saddleback Butte. Let’s talk about the Messier Marathon. The early objects can be tough since they are low in the western
sky and that tends to be too bright and murky just after sunset. Of course the last few objects can be tough, not just because the sun is now rising but by the fact that you must stay up all night to get to them!
Of course about half way through you can “hit the wall”. It’s late, cold and Matt hasn’t brought out the bacon yet and you are now working your way through the dreaded Virgo Cluster. The Virgo cluster of galaxies, in the heart of the Virgo Supercluster comprises some 1500 to 2000 galaxies. So you can see the difficulties of finding a handful of Messier objects that all look just like the other 2000!
If you can make it through the Virgo cluster then you’ve earned your reward. Not only do you get bacon from Matt and coffee from Frank but soon Ophiuchus, Sagittarius and all those lovely globular clusters are on the rise!
Of course, you could just come out for the cookout and just enjoy the company of fellow AVAC members so let’s hope for clear skies and no wind!
Secretary Rose Moore
We have sign-ups started for the Poppy Festival and for the Teens Group Star Party at Edwards for the month of April. Please sign up if you can attend and help out at either event. The Poppy Festival is the weekend of April 18-19, and you can sign up for a couple of hours or more to help out at the booth. The Edwards event is on Friday, April 24th and
is an evening star party.
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Sign-ups for the Mt. Wilson trip for the 100 inch scope will start at May's meeting. You must be a member to sign up, and payment is due when you sign. There will be no online sign-ups or payments. There will be a stand by list for members who are not sure they want to attend, or for non members. Unfortunately, there are only 18 slots. If you are signing up for people who are not at the meeting, they must go on the standby list!
Other items of importance: children must be at least 12; the facilities are not ADA compliant for those who are handicapped; the telescope is at an elevation of 5700 feet - so is not recommended to those with heart or lung issues; smoking is not permitted at Mt. Wilson; climbing stairs is needed to reach the scope.
If any questions, please contact me, Thanks, Rose
Space Place
The heavyweight champion of the Cosmos By Dr. Ethan Siegel As crazy as it once seemed, we once assumed that the Earth was the largest thing in all the universe.
2,500 years ago, the Greek philosopher Anaxagoras was ridiculed for suggesting that the Sun might be even larger than the Peloponnesus peninsula, about 16% of modern-day Greece. Today, we know that planets are dwarfed by stars, which themselves are bound together by the billions or even trillions into galaxies.
But gravitationally bound structures extend far beyond galaxies, which themselves can bind together into massive clusters across the cosmos. While dark energy may be driving most galaxy clusters apart from one another, preventing our local group from falling into the Virgo Cluster, for example, on occasion, huge galaxy clusters can merge, forming the largest gravitationally bound structures in the universe.
Take the "El Gordo" galaxy cluster, catalogued as ACT-CL J0102-4915. It’s the largest known galaxy cluster in the distant universe. A galaxy like the Milky Way might contain a few hundred billion stars and up to just over a trillion (1012) solar masses worth of matter, the El Gordo cluster has an estimated mass of 3 × 1015 solar masses, or 3,000 times as much as our own galaxy! The way we've figured this out is fascinating. By seeing how the shapes of background galaxies are distorted into more elliptical-than-average shapes along a particular set of axes, we can reconstruct how much mass is present in the cluster: a phenomenon known as weak gravitational lensing.
That reconstruction is shown in blue, but doesn't match up with where the X-rays are, which are shown in pink! This is because, when galaxy clusters collide, the neutral gas inside heats up to emit X-rays, but the individual galaxies (mostly) and dark matter (completely) pass through one another, resulting in a displacement of the cluster's mass from its center. This has been observed before in objects like the Bullet Cluster, but El Gordo is much younger and farther away.
Image credit: NASA, ESA, J. Jee (UC Davis), J. Hughes (Rutgers U.), F. Menanteau (Rutgers U. and UIUC), C. Sifon (Leiden Observatory), R. Mandelbum (Carnegie Mellon U.), L. Barrientos (Universidad Catolica de Chile), and K. Ng (UC Davis). X-rays are shown in pink from Chandra; the overall matter density is shown in blue, from lensing derived from the Hubble space telescope. 10 billion light-years distant, El Gordo is the most massive galaxy cluster ever found.
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At 10 billion light-years distant, the light reaching us now was emitted more than 7 billion years ago, when the universe was less than half its present age.
It's a good thing, too, because about 6 billion years ago, the universe began accelerating, meaning that El Gordo just might be the largest cosmic heavyweight of all. There's still more universe left to explore, but for right now, this is the heavyweight champion of the distant universe!
Learn more about “El Gordo” here: http://www.nasa.gov/press/2014/april/nasa-hubble-team-finds-monster-el-gordo-galaxy-cluster-bigger-than-thought/
El Gordo is certainly huge, but what about really tiny galaxies? Kids can learn about satellite galaxies at NASA’s Space Place http://spaceplace.nasa.gov/satellite-galaxies/.
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News Headlines
Leonard Nimoy, 'Star Trek's' Spock, dead at 83 Leonard Nimoy, whose portrayal of "Star Trek's" logic-driven, half-human science officer Spock made him an iconic figure to generations, died Friday. He was 83. Nimoy died this morning in Bel Air, California, his son Adam Nimoy told CNN. According to his granddaughter, Madeleine Nimoy, the cause of death was chronic obstructive pulmonary disease. http://www.cnn.com/2015/02/27/entertainment/feat-obit-leonard-nimoy-spock/ Monster Black Hole in Early Universe A supermassive black hole found only a billion years after the Big Bang adds to growing questions about how such black holes grew so quickly. Astronomers have discovered one of the brightest quasars in the early universe. The source, SDSS J010013.02+280225.8, is powered by a supermassive black hole at a redshift of 6.3, meaning that its light left it 12.8 billion years ago. http://www.skyandtelescope.com/astronomy-news/monster-black-hole-in-early-universe-0226201523/ A Solution to the Puzzle of the Origin of Matter in the Universe Most of the laws of nature treat particles and antiparticles equally, but stars and planets are made of particles, or matter, and not antiparticles, or antimatter. That asymmetry, which favors matter to a very small degree, has puzzled scientists for many years. New research by UCLA physicists offers a possible solution to the mystery of the origin of matter in the universe. http://spaceref.com/astronomy/a-solution-to-the-puzzle-of-the-origin-of-matter-in-the-universe.html Close Call! 'Scholz's Star' Grazed Our Solar System 70,000 Years Ago A dim red dwarf and its brown-dwarf companion likely grazed the outer edges of the solar system 70,000 years ago in what scientists say was the closest encounter ever between our sun and another star. http://www.space.com/28611-star-flew-through-solar-system.html NASA’s Magnetospheric Multiscale (MMS) Spacecraft Set for March Blastoff NASA’s first mission dedicated to study the process in nature known as magnetic reconnection undergoing final preparation for launch from Cape Canaveral, Florida in just under two weeks time. The Magnetospheric Multiscale (MMS) mission is comprised of a quartet of identically instrumented observatories aimed at providing the first three-dimensional views of a fundamental process in nature known as magnetic reconnection. http://www.universetoday.com/119095/nasas-magnetospheric-multiscale-mms-spacecraft-set-for-march-blastoff-to-study-earths-magnetic-reconnection-events/#more-119095 Physicists working to understand how and why matter came about Neutrinos, subatomic remnants of the early universe, are high-energy particles that pass at nearly the speed of light through everything -- our planet, our bodies -- while rarely interacting with other matter. Most of them were born in the beginning, nearly 14 billion years ago, though more are continually made in the nuclear reactions of stars, in human-built nuclear reactors and in particle accelerators used for experimentation. http://www.sciencedaily.com/releases/2015/02/150206125117.htm
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March Sky Data
Best time for deep sky observing this month: March 9 through March 23
Mercury sinks into the Sun's glare as March begins, so this is not a good month to observe it.
Venus, is now an evening object appearing a little higher in the sky as the month progresses. So, shining at magnitude -4 all month, it should be easy to spot above the southwestern horizon about one hour after sunset. Its angular size increases a little from 12 to 14 arc seconds during the month while its gibbous phase wanes from 86% to 78%. Mars is getting dimmer as it lags behind us in its larger and slower orbit. Mars sets about two hours after the sun in early March. It is slowly but surely disappearing into the glow of sunset as Earth races ahead of Mars in its orbit. By late March 2015, Mars will set about one and one-half hours after the sun and will be hard to find in the glare of evening twilight.
Jupiter, having reached opposition on the 6th of February, is high in the south in late evening and visible through much of the night. It starts March shining at at magnitude -2.5, dropping slightly to -2.3 as the month progresses. Jupiter is still moving slowly westwards in retrograde motion towards the Beehive Cluster in Cancer. The size of Jupiter's disk falls slightly from 44.5 to 41.6 arc seconds as March progresses.
Saturn rises around midnight this month lying in the constellation Scorpius very close to the left hand star of the 'fan' that marks its head. Its diameter increases from 16.9 to 17.8 arc seconds during the month as its magnitude increases from +0.4 to +0.3. It will be high enough in the south-south-east before dawn to make out the beautiful ring system which has now opened out to ~25 degrees - virtually as open as they ever become.
There are no major meteor-showers in March, but we may see a handful of meteors from the Virginid shower, which is usually active during March and April; they appear to radiate outwards from the constellation of Virgo.
Sun and Moon Rise and Set Date Moonrise Moonset Sunrise Sunset 3/1/2015 14:32 03:42 06:20 17:47 3/5/2015 18:06 06:04 06:15 17:51 3/10/2015 22:38 08:51 06:09 17:55 3/15/2015 02:17 13:03 06:02 17:59 3/20/2015 06:04 18:46 05:55 18:03 3/25/2015 09:50 ------ 05:48 18:07 3/31/2015 15:08 03:33 05:40 18:11
Planet Data
Mar 1 Rise Transit Set Mag Mercury 05:05 10:25 15:43 0.0 Venus 07:37 13:56 20:15 -4.0 Mars 07:26 13:42 19:57 1.3 Jupiter 15:25 22:22 05:20 -2.5 Saturn 00:12 05:24 10:37 0.5
Mar 15 Rise Transit Set Mag Mercury 06:12 11:48 17:21 -0.2 Venus 08:24 15:03 21:42 -4.0 Mars 07:58 14:26 20:53 1.3 Jupiter 15:24 22:22 05:21 -2.5 Saturn 00:17 05:30 10:42 0.4
Mar 31 Rise Transit Set Mag Mercury 06:20 12:24 18:30 -1.0 Venus 08:13 15:14 22:15 -4.0 Mars 07:26 14:08 20:48 1.4 Jupiter 14:17 21:16 04:15 -2.4 Saturn 23:13 04:26 09:38 0.3 Planet, Sun, and Moon data calculated for local time at Lancaster, CA
Full Mar 5
Last Qtr Mar 13
New Mar 20
First Qtr Mar 26
Chart is plotted for the sky on the date and location of the AVAC Star Party at 10PM.
To use the chart, go outside within an hour or so of the time listed and hold it up to the sky. Turn the chart so the direction you are looking is at the bottom of the chart. If you are looking to the south then have 'South horizon' at the lower edge.
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Suggested Observing List The list below contains objects that will be visible on the night of the AVAC Star Party. Since this month is our Messier Marathon the list is the observing order for the night. You can download the order in Excel format at http://www.avastronomyclub.org/docs/marathon_order.xls or Adobe PDF at http://www.avastronomyclub.org/docs/marathon_order.pdf Order Time M # NGC Con R.A. Dec Mag Type Comments 1 M 77 1068 CET 2h 43m 0° 1' 8.8 SG 2 M 74 628 PSC 1h 37m 15° 47' 9.2 S 3 M 33 598 TRI 1h 34m 30° 39' 5.7 SG Pinwheel galaxy 4 M 31 224 AND 0h 43m 41° 16' 3.4 SG Andromeda galaxy 5 M 32 221 AND 0h 43m 40° 52' 8.2 EG 6 M 110 205 AND 0h 40m 41° 41' 8.0 EG 7 M 52 7654 CAS 23h 24m 61° 35' 6.9 OC 8 M 103 581 CAS 1h 33m 60° 42' 7.4 OC 9 M 76 650 PER 1h 42m 51° 34' 11.5 PN The Little Dumbell 11 M 34 1039 PER 2h 42m 42° 47' 5.2 OC 11 M 45 TAU 3h 47m 24° 7' 1.2 OC Pleiades 12 M 79 1904 LEP 5h 24m -24° 33' 8.0 GC 13 M 42 1976 ORI 5h 35m -5° 27' 4.0 DN Great Orion nebula 14 M 43 1982 ORI 5h 35m -5° 16' 9.0 DN 15 M 78 2068 ORI 5h 47m 0° 3' 8.0 DN 16 M 1 1952 TAU 5h 34m 22° 1' 8.4 PN Crab nebula 17 M 35 2168 GEM 6h 09m 24° 20' 5.1 OC 18 M 37 2099 AUR 5h 52m 32° 33' 5.6 OC 19 M 36 1960 AUR 5h 36m 34° 8' 6.0 OC 20 M 38 1912 AUR 5h 29m 35° 50' 6.4 OC 21 M 41 2287 CMA 6h 47m -20° 44' 4.5 OC 22 M 93 2447 PUP 7h 45m -23° 52' 6.2 OC 23 M 47 2422 PUP 7h 37m -14° 30' 4.4 OC 24 M 46 2437 PUP 7h 42m -14° 49' 6.1 OC 25 M 50 2323 MON 7h 03m -8° 20' 5.9 OC 26 M 48 2548 HYA 8h 14m -5° 48' 5.8 OC 27 M 44 2632 CNC 8h 40m 19° 59' 3.1 OC Beehive Cluster 28 M 67 2682 CNC 8h 50m 11° 49' 6.9 OC 29 M 95 3351 LEO 10h 44m 11° 42' 9.7 SG 30 M 96 3368 LEO 10h 47m 11° 49' 9.2 SG 31 M 105 3379 LEO 10h 48m 12° 35' 9.3 EG 32 M 65 3623 LEO 11h 19m 13° 5' 9.3 SG Leo's triplet 33 M 66 3627 LEO 11h 20m 12° 59' 9.0 SG Leo's triplet 34 M 81 3031 UMA 9h 56m 69° 4' 6.8 SG Bodes Galaxy 35 M 82 3034 UMA 9h 56m 69° 41' 8.4 IG Cigar Galaxy 36 M 97 3587 UMA 11h 15m 55° 1' 11.2 PN Owl Nebula 37 M 108 3556 UMA 11h 12m 55° 40' 10.0 SG
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Order Time M # NGC Con R.A. Dec Mag Type Comments 38 M 109 3992 UMA 11h 58m 53° 23' 9.8 SG 39 M 40 UMA 12h 22m 58° 5' 8.0 dbl 40 M 106 4258 CVN 12h 19m 47° 18' 8.3 SG 41 M 94 4736 CVN 12h 51m 41° 7' 8.1 SG 42 M 63 5055 CVN 13h 16m 42° 2' 8.6 SG Sunflower galaxy 43 M 51 5194 CVN 13h 30m 47° 12' 8.1 SG Whirlpool galaxy 44 M 101 5457 UMA 14h 03m 54° 21' 7.7 SG 45 M 102 5457 UMA 14h 03m 54° 21' 7.7 SG Duplicate of M101 46 M 53 5024 COM 13h 13m 18° 10' 7.7 GC 47 M 64 4826 COM 12h 57m 21° 41' 8.5 SG Black eye galaxy 48 M 3 5272 CVN 13h 42m 28° 23' 6.4 GC 49 M 98 4192 COM 12h 14m 14° 54' 10.1 SG 50 M 85 4382 COM 12h 25m 18° 11' 9.2 EG 51 M 99 4254 COM 12h 19m 14° 25' 9.8 SG Pin Wheel nebula 52 M 100 4321 COM 12h 23m 15° 49' 9.4 SG 53 M 84 4374 VIR 12h 25m 12° 53' 9.3 EG 54 M 86 4406 VIR 12h 26m 12° 57' 9.2 EG 55 M 87 4486 VIR 12h 31m 12° 24' 8.6 EG 56 M 89 4552 VIR 12h 36m 12° 33' 9.8 EG 57 M 90 4569 VIR 12h 37m 13° 10' 9.5 SG 58 M 88 4501 COM 12h 32m 14° 25' 9.5 SG 59 M 91 4548 COM 12h 35m 14° 30' 10.2 SG 60 M 58 4579 VIR 12h 38m 11° 49' 9.8 SG 61 M 59 4621 VIR 12h 42m 11° 39' 9.8 EG 62 M 60 4649 VIR 12h 44m 11° 33' 8.8 EG 63 M 49 4472 VIR 12h 30m 8° 0' 8.4 EG 64 M 61 4303 VIR 12h 22m 4° 28' 9.7 SG 65 M 104 4594 VIR 12h 40m -11° 37' 8.3 SG Sombrero galaxy 66 M 68 4590 HYA 12h 40m -26° 45' 8.2 GC 67 M 83 5236 HYA 13h 38m -29° 52' 7.6 SG Southern Pinwheel 68 M 5 5904 SER 15h 18m 2° 5' 5.8 GC 69 M 13 6205 HER 16h 42m 36° 28' 5.9 GC Hercules Cluster 70 M 92 6341 HER 17h 17m 43° 8' 6.5 GC 71 M 57 6720 LYR 18h 54m 33° 2' 9.0 PN Ring nebula 72 M 56 6779 LYR 19h 17m 30° 11' 8.2 GC 73 M 29 6913 CYG 20h 23m 38° 32' 6.6 OC 74 M 39 7092 CYG 21h 32m 48° 26' 4.6 OC 75 M 27 6853 VUL 20h 00m 22° 43' 8.1 PN Dumbbell nebula 76 M 71 6838 SGE 19h 54m 18° 47' 8.3 GC 77 M 107 6171 OPH 16h 33m -13° 3' 8.1 GC 78 M 10 6254 OPH 16h 57m -4° 6' 6.6 GC 79 M 12 6218 OPH 16h 47m -1° 57' 6.6 GC 80 M 14 6402 OPH 17h 38m -3° 15' 7.6 GC 81 M 9 6333 OPH 17h 19m -18° 31' 7.9 GC 82 M 4 6121 SCO 16h 23m -26° 32' 5.9 GC
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Order Time M # NGC Con R.A. Dec Mag Type Comments 83 M 80 6093 SCO 16h 17m -22° 59' 7.2 GC 84 M 19 6273 OPH 17h 03m -26° 16' 7.2 GC 85 M 62 6266 OPH 17h 01m -30° 7' 6.6 GC 86 M 6 6405 SCO 17h 40m -32° 13' 4.2 OC Butterfly cluster 87 M 7 6475 SCO 17h 54m -34° 49' 3.3 OC Ptolemy's Cluster 88 M 11 6705 SCT 18h 51m -6° 16' 5.8 OC Wild Duck cluster 89 M 26 6694 SGR 18h 45m -9° 24' 8.0 OC 90 M 16 6611 SER 18h 19m -13° 47' 6.0 DN Eagle nebula 91 M 17 6618 SGR 18h 21m -16° 11' 7.0 DN Swan nebula 92 M 18 6613 SGR 18h 20m -17° 8' 6.9 OC 93 M 24 6603 SGR 18h 16m -18° 29' 4.5 OC 94 M 25 SGR 18h 32m -19° 15' 4.6 OC 95 M 23 6494 SGR 17h 57m -19° 1' 5.5 OC 96 M 21 6531 SGR 18h 05m -22° 30' 5.9 OC 97 M 20 6514 SGR 18h 02m -23° 2' 8.5 DN Trifid nebula 98 M 8 6523 SGR 18h 03m -24° 23' 5.8 DN Lagoon nebula 99 M 28 6626 SGR 18h 25m -24° 52' 6.9 GC 100 M 22 6656 SGR 18h 36m -23° 54' 5.1 GC 101 M 69 6637 SGR 18h 31m -32° 21' 7.7 GC 102 M 70 6681 SGR 18h 43m -32° 18' 8.1 GC 103 M 54 6715 SGR 18h 55m -30° 29' 7.7 GC 104 M 55 6809 SGR 19h 40m -30° 58' 7.0 GC 105 M 75 6864 SGR 20h 06m -21° 55' 8.6 GC 106 M 15 7078 PEG 21h 30m 12° 10' 6.4 GC 107 M 2 7089 AQR 21h 33m 0° -49' 6.5 GC 108 M 72 6981 AQR 20h 54m -12° 32' 9.4 GC 109 M 73 6994 AQR 20h 58m -12° 38' ast 110 M 30 7099 CAP 21h 40m -23° 11' 7.5 GC
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A.V.A.C. Information Membership in the Antelope Valley Astronomy Club is open to any individual or family.
The Club has three categories of membership. • Family membership at $30.00 per year. • Individual membership at $25.00 per year. • Junior membership at $15.00 per year.
Membership entitles you to… • Desert Sky Observer–monthly newsletter. • The Reflector – the publication of the Astronomical League. • The A.V.A.C. Membership Manual. • To borrow club equipment, books, videos and other items.
AVAC P.O. BOX 8545, LANCASTER, CA 93539-8545 Visit the Antelope Valley Astronomy Club website at www.avastronomyclub.org/
The Antelope Valley Astronomy Club, Inc. is a 501(c)(3) Non-Profit Corporation.
The A.V.A.C. is a Sustaining Member of The Astronomical League and the International Dark-Sky Association.
Board Members President:
Frank Moore (661) 972-4775 [email protected]
Vice-President: Don Bryden (661) 270-0627 [email protected]
Secretary: Rose Moore (661) 972-1953 [email protected]
Treasurer: Virgina Reed (661) 824-3932 [email protected]
Director of Community Development: Robert Lynch, Jr. [email protected]
Appointed Positions Newsletter Editor:
Steve Trotta (661) 269-5428 [email protected]
Equipment & Library: Bill Grove [email protected]
Club Historian: Tom Koonce (661) 943-8200 [email protected]
Webmaster: Steve Trotta (661) 269-5428 [email protected]
Astronomical League Coordinator: Don Bryden (661) 270-0627 [email protected]
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Our Sponsors Thank you to our sponsors for your generous support!
Cosmos Level Sponsors
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5348 Topanga Canyon Blvd., Woodland Hills 888-427-8766.
www.telescopes.net
Universe Level Sponsors
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